Measuring the chemical composition of cosmic rays at ? 1013?1015 eV by utilizing the solar and geomagnetic fields-Reference-Cited by-同舟云学术

Measuring the chemical composition of cosmic rays at ? 1013?1015 eV by utilizing the solar and geomagnetic fields

Author:

Heintze J.,Lennert P.,Polenz S.,Schmidt B.,Spitzer J.,Br�ckner W.,Hofmann W.,Povh B.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

Reference7 articles.

1. Gaisser, T.K. and Stanev, T., private communication

3. Heintze, J. et al. (1988). Heidelberg-Rep., HD-PY 88/05, to appear in Nucl. Inst. and Methods

4. Khristiansen, G.B. (1987). Proc. 20th ICRC, Moskow, Vol.8, p.54

5. Lloyd-Evans, J. (1985). Proc. 19th ICRC, La Jolla, Vol.2, p.173

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3. Cosmic ray tracking: a new approach to high-energy γ-astronomy;Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment;1991-12

4. A method to measure the γ-ray content in VHE cosmic ray showers;Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment;1991-09